{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:FAGWWSBLYCOOND2L3QKXVXHR3X","short_pith_number":"pith:FAGWWSBL","schema_version":"1.0","canonical_sha256":"280d6b482bc09ce68f4bdc157adcf1ddf32c05099f058f7a8ad5c3c1b15fb546","source":{"kind":"arxiv","id":"1410.7198","version":2},"attestation_state":"computed","paper":{"title":"Deep Washington photometry of inconspicuous star cluster candidates in the Large Magellanic Cloud","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Andr\\'es E. Piatti, Annapurni Subramaniam, Samyaday Choudhury","submitted_at":"2014-10-27T12:11:21Z","abstract_excerpt":"We present deep Washington photometry of 45 poorly populated star cluster candidates in the Large Magellanic Cloud (LMC). We have performed a systematic study to estimate the parameters of the cluster candidates by matching theoretical isochrones to the cleaned and de-reddened cluster color-magnitude diagrams (CMDs). We were able to estimate the basic parameters for 33 clusters, out of which, 23 are identified as single clusters and 10 are found to be members of double clusters. Other 12 cluster candidates have been classified as possible clusters/asterisms. About 50% of the true clusters are "},"verification_status":{"content_addressed":true,"pith_receipt":true,"author_attested":false,"weak_author_claims":0,"strong_author_claims":0,"externally_anchored":false,"storage_verified":false,"citation_signatures":0,"replication_records":0,"graph_snapshot":true,"references_resolved":false,"formal_links_present":false},"canonical_record":{"source":{"id":"1410.7198","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2014-10-27T12:11:21Z","cross_cats_sorted":[],"title_canon_sha256":"9ef2031eb9199aaad9ac9e53496e1bf4d631b1c1d5e94ccfafbd7c02f49e20e2","abstract_canon_sha256":"a01ca209f8acc7187f931f1d52794844cc880d14b6191b0db3fa30ef11cd36be"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:41:39.718395Z","signature_b64":"j4OuSXDTBKNmPTAE0E/N0bPJYdhz17DI7Hzem5Y1UxNeMIoG/oKgqKtgl7haxHnqTdQHJh61VQUmU22t4Y0wDQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"280d6b482bc09ce68f4bdc157adcf1ddf32c05099f058f7a8ad5c3c1b15fb546","last_reissued_at":"2026-05-18T01:41:39.717916Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:41:39.717916Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Deep Washington photometry of inconspicuous star cluster candidates in the Large Magellanic Cloud","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Andr\\'es E. Piatti, Annapurni Subramaniam, Samyaday Choudhury","submitted_at":"2014-10-27T12:11:21Z","abstract_excerpt":"We present deep Washington photometry of 45 poorly populated star cluster candidates in the Large Magellanic Cloud (LMC). We have performed a systematic study to estimate the parameters of the cluster candidates by matching theoretical isochrones to the cleaned and de-reddened cluster color-magnitude diagrams (CMDs). We were able to estimate the basic parameters for 33 clusters, out of which, 23 are identified as single clusters and 10 are found to be members of double clusters. Other 12 cluster candidates have been classified as possible clusters/asterisms. About 50% of the true clusters are "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1410.7198","kind":"arxiv","version":2},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"},"aliases":[{"alias_kind":"arxiv","alias_value":"1410.7198","created_at":"2026-05-18T01:41:39.717983+00:00"},{"alias_kind":"arxiv_version","alias_value":"1410.7198v2","created_at":"2026-05-18T01:41:39.717983+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1410.7198","created_at":"2026-05-18T01:41:39.717983+00:00"},{"alias_kind":"pith_short_12","alias_value":"FAGWWSBLYCOO","created_at":"2026-05-18T12:28:28.263976+00:00"},{"alias_kind":"pith_short_16","alias_value":"FAGWWSBLYCOOND2L","created_at":"2026-05-18T12:28:28.263976+00:00"},{"alias_kind":"pith_short_8","alias_value":"FAGWWSBL","created_at":"2026-05-18T12:28:28.263976+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/FAGWWSBLYCOOND2L3QKXVXHR3X","json":"https://pith.science/pith/FAGWWSBLYCOOND2L3QKXVXHR3X.json","graph_json":"https://pith.science/api/pith-number/FAGWWSBLYCOOND2L3QKXVXHR3X/graph.json","events_json":"https://pith.science/api/pith-number/FAGWWSBLYCOOND2L3QKXVXHR3X/events.json","paper":"https://pith.science/paper/FAGWWSBL"},"agent_actions":{"view_html":"https://pith.science/pith/FAGWWSBLYCOOND2L3QKXVXHR3X","download_json":"https://pith.science/pith/FAGWWSBLYCOOND2L3QKXVXHR3X.json","view_paper":"https://pith.science/paper/FAGWWSBL","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1410.7198&json=true","fetch_graph":"https://pith.science/api/pith-number/FAGWWSBLYCOOND2L3QKXVXHR3X/graph.json","fetch_events":"https://pith.science/api/pith-number/FAGWWSBLYCOOND2L3QKXVXHR3X/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/FAGWWSBLYCOOND2L3QKXVXHR3X/action/timestamp_anchor","attest_storage":"https://pith.science/pith/FAGWWSBLYCOOND2L3QKXVXHR3X/action/storage_attestation","attest_author":"https://pith.science/pith/FAGWWSBLYCOOND2L3QKXVXHR3X/action/author_attestation","sign_citation":"https://pith.science/pith/FAGWWSBLYCOOND2L3QKXVXHR3X/action/citation_signature","submit_replication":"https://pith.science/pith/FAGWWSBLYCOOND2L3QKXVXHR3X/action/replication_record"}},"created_at":"2026-05-18T01:41:39.717983+00:00","updated_at":"2026-05-18T01:41:39.717983+00:00"}